- ID:
- ivo://wfau.roe.ac.uk/atlasDR1-dsa
- Title:
- ATLAS DR1 - VST ATLAS Survey
- Date:
- 23 Jan 2024 09:42:24
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 1 of the ATLAS Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands. The ATLAS will complement the proposed VISTA Hemisphere Survey in the South.
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- ID:
- ivo://cxc.harvard.edu/csc
- Title:
- Chandra Source Catalog
- Short Name:
- CSC
- Date:
- 24 Oct 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory and one of NASA"s Great Observatories. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. The Chandra Source Catalog (CSC) includes information about X-ray sources detected in observations obtained using the Chandra X-ray Observatory. Release 2.0 of the catalog includes 317,167 point, compact, and extended sources detected in ACIS and HRC-I imaging observations released publicly prior to the end of 2014. Observed source positions and multi-band count rates are reported, as well as numerous derived spatial, photometric, spectral, and temporal calibrated source properties that may be compared with data obtained by other telescopes. Each record includes the best estimates of the properties of a source based on data extracted from all observations in which the source was detected. The Chandra Source Catalog is extracted from the CXC"s Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. For detailed information on the Chandra Observatory and datasets see: http://cxc.harvard.edu/ for general Chandra information; http://cxc.harvard.edu/cda/ for the Chandra Data Archive; http://cxc.harvard.edu/csc/ for Chandra Source Catalog information.
- ID:
- ivo://cxc.harvard.edu/cscr1
- Title:
- Chandra Source Catalog Release 1
- Short Name:
- CSCR1
- Date:
- 24 Oct 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory and one of NASA"s Great Observatories. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. The Chandra Source Catalog (CSC) includes information about X-ray sources detected in observations obtained using the Chandra X-ray Observatory. Release 1.1 of the catalog includes about 138,000 point and compact sources with observed spatial extents less than ~30 arcsec detected in a subset of ACIS and HRC-I imaging observations released publicly prior to the end of 2009. Observed source positions and multi-band count rates are reported, as well as numerous derived spatial, photometric, spectral, and temporal calibrated source properties that may be compared with data obtained by other telescopes. Each record includes the best estimates of the properties of a source based on data extracted from all observations in which the source was detected. The Chandra Source Catalog is extracted from the CXC"s Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. For detailed information on the Chandra Observatory and datasets see: http://cxc.harvard.edu/ for general Chandra information; http://cxc.harvard.edu/cda/ for the Chandra Data Archive; http://cxc.harvard.edu/csc/ for Chandra Source Catalog information.
- ID:
- ivo://cxc.harvard.edu/cscr2
- Title:
- Chandra Source Catalog Release 2
- Short Name:
- CSCR2
- Date:
- 24 Oct 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory and one of NASA"s Great Observatories. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. The Chandra Source Catalog (CSC) includes information about X-ray sources detected in observations obtained using the Chandra X-ray Observatory. Release 2.0 of the catalog includes 317,167 point, compact, and extended sources detected in ACIS and HRC-I imaging observations released publicly prior to the end of 2014. Observed source positions and multi-band count rates are reported, as well as numerous derived spatial, photometric, spectral, and temporal calibrated source properties that may be compared with data obtained by other telescopes. Each record includes the best estimates of the properties of a source based on data extracted from all observations in which the source was detected. The Chandra Source Catalog is extracted from the CXC"s Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. For detailed information on the Chandra Observatory and datasets see: http://cxc.harvard.edu/ for general Chandra information; http://cxc.harvard.edu/cda/ for the Chandra Data Archive; http://cxc.harvard.edu/csc/ for Chandra Source Catalog information.
- ID:
- ivo://cxc.harvard.edu/cda
- Title:
- Chandra X-ray Observatory Data Archive
- Short Name:
- CDA
- Date:
- 18 Jul 2019
- Publisher:
- Chandra X-ray Observatory
- Description:
- The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory. Chandra was formerly known as AXAF, the Advanced X-ray Astrophysics Facility, but renamed by NASA in December, 1998. Originally three instruments and a high-resolution mirror carried in one spacecraft, the project was reworked in 1992 and 1993. The Chandra spacecraft carries a high resolution mirror, two imaging detectors, and two sets of transmission gratings. Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range.
- ID:
- ivo://mssl.ucl.ac.uk/chianti_dsa/chianti
- Title:
- Chianti Data Set
- Date:
- 16 Sep 2009 16:04:57
- Publisher:
- Mullard Space Science Laboratory
- Description:
- CHIANTI consists of a critically evaluated set of up-to-date atomic data
- ID:
- ivo://helio-vo.eu/cxs
- Title:
- Context Service
- Short Name:
- CXS
- Date:
- 29 Aug 2014 10:35:00
- Publisher:
- HELIO
- Description:
- Execution service - implemented in the Common Execution Architecture - that generates context information on-demand. This service provides one or more science applications that are registered separately
- ID:
- ivo://helio-vo.eu/cts
- Title:
- Coordinate Transformation Service
- Short Name:
- CTS
- Date:
- 26 Jun 2014 13:21:29
- Publisher:
- HELIO
- Description:
- Service that performs transformation between coordinate sets. Service is implemented in the Common Execution Architecture and is in fact part of the CXS.
- ID:
- ivo://au.csiro/casda/SCS
- Title:
- CSIRO ASKAP Science Data Archive Cone Search Service
- Short Name:
- CSIRO ASKAP Cone
- Date:
- 01 Dec 2023 14:46:51
- Publisher:
- CSIRO
- Description:
- Cone search service for querying catalogues from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/casda/SIA2
- Title:
- CSIRO ASKAP Science Data Archive Image Access Service
- Short Name:
- CSIRO ASKAP SIA2
- Date:
- 07 Jul 2017 16:23:19
- Publisher:
- CSIRO
- Description:
- Simple Image Access v2 service for querying multi-dimensional image products from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/casda/SSA
- Title:
- CSIRO ASKAP Science Data Archive Spectrum Access Service
- Short Name:
- CSIRO ASKAP SSA
- Date:
- 29 Apr 2022 07:59:11
- Publisher:
- CSIRO
- Description:
- Simple Spectral Access service for querying spectra from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/casda/TAP
- Title:
- CSIRO ASKAP Science Data Archive TAP Service
- Short Name:
- CSIRO ASKAP TAP
- Date:
- 09 Nov 2018 08:39:00
- Publisher:
- CSIRO
- Description:
- Table Access Protocol service for accessing catalogues from ASKAP radio astronomy observations
- ID:
- ivo://au.csiro/atoavo/TAP
- Title:
- CSIRO Australia Telescope Online Archive TAP Service
- Short Name:
- CSIRO ATOA TAP
- Date:
- 17 Jul 2020 16:23:58
- Publisher:
- CSIRO
- Description:
- Table Access Protocol service for accessing Australia Telescope Online Archive
- ID:
- ivo://au.csiro/psrda/ATNF_Pulsar_Data_Archive
- Title:
- CSIRO Parkes Pulsar Data Archive
- Short Name:
- CSIRO Pulsar TAP
- Date:
- 27 Jun 2018 15:23:26
- Publisher:
- CSIRO
- Description:
- Repository of pulsar observations made at the Parkes, Australia radio telescope
- ID:
- ivo://au.csiro/psrda/ATNF_Pulsar_SCS
- Title:
- CSIRO Parkes Pulsar Data Archive Cone Search Service
- Short Name:
- CSIRO Pulsar SCS
- Date:
- 27 Jun 2018 15:26:24
- Publisher:
- CSIRO
- Description:
- Repository of pulsar observations made at the Parkes, Australia radio telescope
- ID:
- ivo://mssl.ucl.ac.uk/solar_events_dsa/Solar_Event_Catalogue
- Title:
- Datacenter for Solar Event Catalogue
- Date:
- 11 Aug 2009 14:42:11
- Publisher:
- Mullard Space Science Laboratory
- Description:
- Data Set for querying the Solar Event Catalogue (SEC)
- ID:
- ivo://helio-vo.eu/dpas
- Title:
- Data Provider Access Service
- Short Name:
- DPAS
- Date:
- 26 Jun 2014 13:20:17
- Publisher:
- HELIO
- Description:
- Service that acts as an intermediary between the user and data providers.
- ID:
- ivo://wfau.roe.ac.uk/denis-dsa
- Title:
- Deep Near Infrared Survey of the Southern Sky (DENIS)
- Date:
- 04 Dec 2019 13:34:37
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Catalog of astrometry and photometry of detected point sources in the Far red optical (0.82-micron I-band) and near-infrared (1.25-micron J- and 2.15-micron Ks bands). ~16,700 square degrees of the southern sky
- ID:
- ivo://wfau.roe.ac.uk/6df-dsa
- Title:
- 6dF Galaxy Survey Data Release 2
- Short Name:
- 6dF DR2
- Date:
- 23 Jan 2024 09:39:52
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75).
- ID:
- ivo://wfau.roe.ac.uk/6dfdr3-dsa
- Title:
- 6dF Galaxy Survey Data Release 3
- Short Name:
- 6dF DR3
- Date:
- 23 Jan 2024 09:38:59
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75). This is the Data Release 3 version.
- ID:
- ivo://wfau.roe.ac.uk/first-dsa
- Title:
- FIRST Survey Catalogue (03Apr11 Version)
- Short Name:
- FIRST
- Date:
- 04 Dec 2019 13:34:53
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- FIRST (Faint Images of the Radio Sky at Twenty-cm) is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North and South Galactic Caps. The catalogue covers a total of about 9033 square degrees of sky (8422 square degrees in the north Galactic cap and 611 square degrees in the south Galactic cap.)
22. GALEX Release 6
- ID:
- ivo://wfau.roe.ac.uk/galexgr6-dsa
- Title:
- GALEX Release 6
- Date:
- 23 Jan 2024 09:43:10
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy
- ID:
- ivo://nasa.heasarc/services/xamin
- Title:
- HEASARC Xamin Catalog Interface
- Short Name:
- HEASARC
- Date:
- 21 Mar 2017
- Publisher:
- NASA/GSFC HEASARC
- Description:
- The HEASARC is NASA domain archive for high-energy and microwave astronomy. The Xamin interface provides access to over 600 observation and object tables. This includes observation tables for more than 30 missions and observatories and hundreds of derived object tables. Non-high energy tables are included to make it easier for users to compare information.
- ID:
- ivo://helio-vo.eu/hec
- Title:
- Heliophysics Event Catalogue
- Short Name:
- HEC
- Date:
- 29 Jan 2018 15:53:51
- Publisher:
- HELIO
- Description:
- Database of lists of events from various heliophysical domains
- ID:
- ivo://helio-vo.eu/hec/trieste
- Title:
- Heliophysics Event Catalogue in Trieste
- Date:
- 26 Jul 2012 07:02:39
- Publisher:
- INAF
- Description:
- Heliophysics Event Catalogue Description
- ID:
- ivo://helio-vo.eu/hec/turin
- Title:
- Heliophysics Event Catalogue in Turin
- Date:
- 25 Feb 2014 14:14:46
- Publisher:
- INAF
- Description:
- Heliophysics Event Catalogue Description
- ID:
- ivo://helio-vo.eu/hfc
- Title:
- Heliophysics Feature Catalogue
- Short Name:
- HFC
- Date:
- 21 May 2015 16:33:30
- Publisher:
- HELIO
- Description:
- Database describing features from various heliophysical domains
- ID:
- ivo://mssl.ucl.ac.uk/hinode_dsa/hinode
- Title:
- Hinode EIS Level 0 and Level 2
- Date:
- 11 Aug 2009 15:09:22
- Publisher:
- Mullard Space Science Laboratory
- Description:
- Hinode Data set access
- ID:
- ivo://wfau.roe.ac.uk/iras-dsa
- Title:
- Infrared Astronomical Satellite Archive (IRAS)
- Short Name:
- IRAS
- Date:
- 04 Dec 2019 13:35:12
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Infrared Astronomical Satellite Archive is an implementation of the IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986). This is a catalogue of some 250,000 well-confirmed infrared point sources observed by the Infrared Astronomical Satellite, i.e., sources with angular extents less than approximately 0.5, 0.5, 1.0, and 2.0 arcmin in the in-scan direction at 12, 25, 60, and 100 microns, respectively.
- ID:
- ivo://helio-vo.eu/ics
- Title:
- Instrument Capability Service
- Short Name:
- ICS
- Date:
- 21 Aug 2014 11:58:58
- Publisher:
- HELIO
- Description:
- Database describing the capabilities of instruments that could be accessed by HELIO
- ID:
- ivo://helio-vo.eu/ils
- Title:
- Instrument Location Service
- Short Name:
- ILS
- Date:
- 21 Aug 2014 11:52:01
- Publisher:
- HELIO
- Description:
- Database of the location of observatories and planets
- ID:
- ivo://wfau.roe.ac.uk/twompz-dsa
- Title:
- 2MASS Photometric Redshift catalogue (2MPZ)
- Date:
- 23 Jan 2024 09:45:12
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 2MASS Photometric Redshift catalogue (2MPZ) is constructed by cross-matching 2MASS XSC, WISE and SuperCOSMOS all-sky samples and employing the artificial neural network approach (the ANNz algorithm, Collister & Lahav 2004), trained on several redshift surveys (2MRS, SDSS, 6dFGS, 2dFGRS and ZCAT). The derived photometric redshifts have errors nearly independent of distance, with an all-sky accuracy of Ïz = 0.015, and a very small percentage of outliers. These redshift estimates have a typical precision of 12% for all the 2MASS XSC galaxies that lack spectroscopy. The resulting 2MPZ sample contains almost 1 million galaxies with a median redshift of z=0.07. This catalogue is described in Bilicki et al. 2014, ApJS, 210, 9.
- ID:
- ivo://wfau.roe.ac.uk/mgc-dsa
- Title:
- Millennium Galaxy Catalogue (MGC)
- Date:
- 04 Dec 2019 13:35:24
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Millennium Galaxy Catalogue (MGC) is a 37.5 deg2, medium-deep, B-band imaging survey obtained with the Wide Field Camera on the INT. The survey region is a long, 35 arcmin wide strip along the equator, covering from 10h 00m to 14h 45m and is fully contained within the regions of both the Two Degree Field Galaxy Redshift Survey (2dFGRS) and the Sloan Digital Sky Survey (SDSS).
34. MSSL CEA service
- ID:
- ivo://mssl.ucl.ac.uk/MSSLToolCEAAccess
- Title:
- MSSL CEA service
- Short Name:
- MSSL-CEA
- Date:
- 11 Aug 2009 14:59:15
- Publisher:
- AstroGrid
- Description:
- A service in the Common Execution Architecture. This service provides one or more science applications which are separately registered. See the ManagedApplications element of this document for a list of applications.
35. MSSL Community
- ID:
- ivo://mssl.ucl.ac.uk/community
- Title:
- MSSL Community
- Date:
- 11 Jun 2008 10:47:43
- Publisher:
- MSSL
- Description:
- This resource describes the community webapplication at MSSL. It hosts all the accounts and secure accounts of people organized at MSSL. And possibly other outside people of MSSL but associated with projects of MSSL.
- ID:
- ivo://wfau.roe.ac.uk/osa-tap
- Title:
- OSA VST ATLAS Survey
- Short Name:
- WFAU OSA TAP
- Date:
- 28 May 2018 17:35:25
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This service hosts the public releases of the ATLAS Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh, as well as a number of other external datasets for which WFAU has neighbour tables, that can be cross matched with ATLAS. The initial aim of ATLAS is to survey 4500 deg2 of the Southern Sky at high galactic latitudes to comparable depths to the SDSS in the North. The VST ATLAS will be the first step towards a panoramic digital survey of the Southern Sky in the optical bands. The ATLAS will complement the proposed VISTA Hemisphere Survey in the South.
- ID:
- ivo://wfau.roe.ac.uk/pssa-dsa
- Title:
- Personal SuperCOSMOS Science Archive (SSA)
- Date:
- 23 Jan 2024 09:43:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- Small subset of the SuperCOSMOS Science Archive, useful for testing queries. The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
- ID:
- ivo://wfau.roe.ac.uk/rosat-dsa
- Title:
- Rontgen Satellite Archive (ROSAT)
- Short Name:
- ROSAT
- Date:
- 04 Dec 2019 13:35:43
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Rontgen Satellite Archive is an implementation of the ROSAT All-Sky Survey Bright Source Catalogue (RASS-BSC, revision 1RXS) and the ROSAT All-Sky Survey Faint Source Catalogue (RASS-FSC, revision 1RXS). The RASS-BSC is derived from the all-sky survey performed during the first half year of the ROSAT mission in 1990/91. 18,811 sources are catalogued, with a limiting ROSAT PSPC countrate of 0.05 cts/s in the 0.1-2.4 keV energy band. The sources have a detection likelihood of at least 15 and contain at least 15 source photons. At a brightness limit of 0.1 cts/s (8,547 sources) the catalogue represents a sky coverage of 92%. The typical positional accuracy is 30 arcsec. The RASS-FSC is derived from the all-sky survey performed during the ROSAT mission in the energy band 0.1- 2.4 keV. 105,924 sources are catalogued and represent the faint extension to the RASS bright source catalogue. The sources have a detection likelihood of at least 7 and contain at least 6 source photons. (The likelihood of source detection is defined as L =-ln (1-P) , with P = probability of source detection).
- ID:
- ivo://sao.ru/community
- Title:
- SAO of RAS community service
- Date:
- 20 Apr 2011 14:56:44
- Publisher:
- SAO of RAS
- Description:
- ID:
- ivo://wfau.roe.ac.uk/sdssdr5-dsa
- Title:
- SDSS DR5 - Sloan Digital Sky Survey Data Release 5
- Short Name:
- SDSS DR5
- Date:
- 04 Dec 2019 13:36:06
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR5 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr3-dsa
- Title:
- SDSS DR3 - Sloan Digital Sky Survey Data Release 3
- Short Name:
- SDSS DR3
- Date:
- 04 Dec 2019 13:35:52
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR3 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr9-dsa
- Title:
- SDSS DR9 - Sloan Digital Sky Survey Data Release 9
- Date:
- 04 Dec 2019 13:36:43
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR9 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr8-dsa
- Title:
- SDSS DR8 - Sloan Digital Sky Survey Data Release 8
- Short Name:
- SDSS DR8
- Date:
- 04 Dec 2019 13:36:31
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR8 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://wfau.roe.ac.uk/sdssdr7-dsa
- Title:
- SDSS DR7 - Sloan Digital Sky Survey Data Release 7
- Short Name:
- SDSS DR7
- Date:
- 04 Dec 2019 13:36:17
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This is an AstroGrid Dataset Access installation of the Sloan Digital Sky Survey (SDSS) DR7 hosted by the Wide Field Astronomy Unit (WFAU), University of Edinburgh. WFAU would like to thank John Hopkins University and the University of Chicago for permission to host the data.
- ID:
- ivo://mssl.ucl.ac.uk/solarimg_dsa/solarimg
- Title:
- Solar Image Data for EIT CDS and Yohkoh
- Date:
- 11 Aug 2009 14:38:28
- Publisher:
- Mullard Space Science Laboratory
- Description:
- Catalogues of solar observations held at MSSL/UCL. Datasets available are SOHO CDS, SOHO EIT, Yohkoh SXT. URL links to data files are provided (EIT data files provided by SDAC, NASA). Reference: http://www.mssl.ucl.ac.uk/www_solar/surfindex.html
- ID:
- ivo://sao.ru/dsa-cats/wsdb
- Title:
- Special Astrophysical Observatory of RAS (SAO RAS) DSA-Catalogs Service
- Date:
- 14 Aug 2019 16:16:36
- Publisher:
- Special Astrophysical Observatory of RAS (SAO RAS)
- Description:
- The published catalogs of Special Astrophysical Observatory of RAS (SAO RAS)
- ID:
- ivo://wfau.roe.ac.uk/ssa-dsa
- Title:
- SuperCOSMOS Science Archive (SSA)
- Short Name:
- SuperCOSMOS
- Date:
- 23 Jan 2024 09:44:26
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The SuperCOSMOS data held in the SSA primarily originate from scans of Palomar and UK Schmidt blue, red and near-IR southern sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide a 1st epoch red measurement. Further details on the surveys, the scanning process and the raw parameters extracted can be found on the further information link. The SSA is housed in a relational database running on Microsoft SQL Server 2000. Data are stored in tables which are inter-linked via reference ID numbers. In addition to the astronomical object catalogues these tables also contain information on the plates that were scanned, survey field centres and calibration coefficients. Most user science queries will only need to access the SOURCE table or to a lesser extent the DETECTION table.
- ID:
- ivo://wfau.roe.ac.uk/twomass-dsa
- Title:
- Two Micron All Sky Survey (2MASS)
- Short Name:
- 2MASS
- Date:
- 04 Dec 2019 13:36:55
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The Two Micron All Sky Survey (2MASS) will provide a uniform survey of the entire sky at three near-infrared wavebands: J(lambdaeff = 1.25 micrometers), H(lambdaeff = 1.65 micrometers), and Ks(lambdaeff = 2.16 micrometers). A major goal of the survey is to probe large scale structures in the Milky Way and in the Local Universe, exploiting the relatively high transparency of the interstellar medium in the near-infrared, and the high near-infrared luminosities of evolved low- and intermediate-mass stars.Home page at http://pegasus.phast.umass.edu/
- ID:
- ivo://wfau.roe.ac.uk/uhsDR2-dsa
- Title:
- UHS DR2 - UKIRT Hemisphere Survey Data Release 2
- Date:
- 23 Jan 2024 09:45:50
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- This DSA hosts data release 2 of the UKIRT Hemisphere Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. The UHS provides continuous J and K-band coverage in the northern hemisphere from a declination of 0 deg to 60 deg.
- ID:
- ivo://wfau.roe.ac.uk/ukidssDR8-v1/UKIDSS_DR8
- Title:
- UKIDSS DR8 (Secure Access)
- Date:
- 06 Oct 2010 16:30:56
- Publisher:
- WFAU
- Description:
- This DSA hosts data release 8 of the UKIRT Infrared Deep Sky Survey housed at the Wide Field Astronomy Unit at the Univeristy of Edinburgh. In order to access this data you need to contact Mark Holliman at msh@roe.ac.uk to be added to the authorized users list. This catalog contains WFCAM data primarily originating from the five UKIDSS surveys: Large Area Survey, Galactic Plane Survey, Galactic Clusters Survey, Deep Extragalactic Survey and the Ultra Deep Survey (see the www.ukidss.org for survey descriptions)